The newly acquired data of HD 80606 b along with the historical measurements for RV, transit and eclipse are analyzed in a self-consistent manner in order to place constraints on the system parameters. The radial velocity observations help constrain the orbit and alignment of HD 80606 b, which is particularly important considering the high eccentricity of the planet can drastically change the transit duration based on the argument of periastron [1]}. The transit observations help the size of the planet once the orbit is reliably known and disentangled from degeneracies involving the stellar radius, inclination and contamination by HD 80607. Additionally, using the measured times of mid-transit and mid-eclipse we can search for deviations from a Keplerian orbit, which is potentially indicative of a companion in the system ([2]}; [3]}).
